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Neutron Scattering

Neutron Scattering - JuSER - Forschungszentrum Jülich

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determination of accurate atomic parameters (positional and thermal parameters, site<br />

occupations) of lighter elements in the presence ofheavy ones .<br />

The contrast in conventional X-ray diffraction is directly related to the ratio ofthe number of<br />

electrons Zj of thé différent atoms or ions j involved . The atomic scattering factor f in thé<br />

structure-factor formula, which represents thé Fourier transform of thé atomic electron<br />

density distribution, is proportional to Zj (f = Zj for sin9/A, = 0) . Standard X-ray techniques<br />

can hardly differentiate between atoms/ions of a similar number of electrons, and only an<br />

average structure - including a total occupation probability of mixed occupied sites - may be<br />

obtained in such cases .<br />

For neutrons thé atomic scattering factor f is replaced by thé nuclear scattering length (or<br />

coherent scattering amplitude) bj, which is ofthé same order of magnitude for all nuclei but<br />

varies from nucleus to nucleus in a non-systematic way . b,, values, which can be either<br />

positive or negative, depend on thé isotopes and nuclear spin states of thé element j . A<br />

nucleus of an isotope with spin I may have two différent neutron scattering lengths : one for<br />

thé combined spin state J = I + %2 and one with J = I - '/z . An important and fundamental<br />

example is provided by thé simplest of all nuclei, thé proton with spin I = 1/2 . The two spin<br />

states, J = 1 (triplet) and J = 0 (singlet), with statistical weights 3/4 and 1/4 respectively, have<br />

thé scattering lengths for afree proton :<br />

b SH=-23 .7 fin, b'H=+5 .38 fin, bfre,H = 1/4b'H + 3/4b'H = -1 .89 lin (with 10 -15 m = 1 lin).<br />

The value for thé bound proton in a ciystal structure, which is to be used in thé structure<br />

factor calculations, amounts to bl, = 2 -bfreeFl = -3 .741 fm.<br />

The natural isotope mixture and a statistical spin-state distribution lead to thé commonly used<br />

general formula bj = with thé sum of thé différent isotope fractions<br />

a+13+y+. . . = 1 (boa, bop, bj,, being thé individual scattering lengths of thé différent isotopes of<br />

thé element j) . The natural nickel isotopes, for instance, have extremely différent coherent<br />

scattering amplitudes :<br />

b( 58Ni) = +14 .4 fin, b(6°Ni) = +3 .0 fin, b(61Ni) = +7 .6 fm,b(62Ni) = -8 .7 fin, b(64Ni) = -0.37 fin<br />

resulting in an overall scattering length bNi = +10 .34 fm .<br />

<strong>Neutron</strong> experiments frequently make use of compounds containing single isotope elements,<br />

like fully deuterated samples . Incoherent scattering due to a statistical distribution of isotopes<br />

and nuclear spin states is not discussed here . It may influence thé effective absorption and thé<br />

background conditions ofneutron diffraction studies .<br />

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